Posted on 12/14/2001 2:39:25 PM PST by grimalkin
The Mars Odyssey (MO) spacecraft has made its first significant discovery: it has detected large deposits of hydrogen - possibly water - near the Red Planet's poles.
Reporting MO's preliminary observations, scientists said the first pass by the probe's neutron spectrometer had revealed evidence of the element in soil at high latitudes.
"It is big," Bill Feldman, of Los Alamos National Laboratory, said of the strength of the signal picked up by Odyssey.
The results indicate large amounts of hydrogen on the surface, a likely sign of water-ice. The observations "are precisely what you would expect for a very hydrogen-rich environment", Feldman said.
Water, water, everywhere?
American space agency (Nasa) scientists said they were excited by the initial indications of hydrogen deposits, describing the readings sent back as clearer, more definite and much earlier than had been expected.
"We were expecting that it would take many orbits to determine the presence of hydrogen," said Stephen Saunders, a MO scientist. "But we saw it the very first time."
Scientists already know that water exists on Mars; it is frozen in the polar icecaps and exists as vapour in thin clouds.
There is also good evidence that water flowed on the planet's surface in the recent past, carving out deep channels and canyons.
Mapping mission
Significant water-ice deposits easily accessible from the surface would make it much more likely that life existed at some stage on Mars.
The MO is currently tightening its orbit around the Red Planet for a mapping mission that will get underway in January. It will use a battery of instruments to survey the planet's surface.
As well as the neutron spectrometer, its gamma-ray spectrometer will chart the chemical composition of the surface. Its infrared camera will peer at areas on the night side of Mars.
"We think it will be a very exciting winter and spring," James Garvin, a Nasa scientist, told a meeting of the American Geophysical Union in San Francisco.
I thought the New World was plundered for its gold and legitimate trade soon followed. I think unmanned probes and space telescopes are paying off with a wealth of knowledge, but the Space Shuttle and Space Station in their current states are nothing but money pits. The 100 billion plus dollars going into them could be better spent on space research that would make the benefits we get from space far greater.
We could be doing far better than that, if only we'd get working on propulsion systems instead of wasting money on low-tech trivia like manned missions to Mars. In this galaxy alone there must be enough usable planets that everyone now on earth could own several. Virtually infinite riches are out there, waiting for us, if we could just figure out how to get there. Plenty of incentive, but too much bureaucracy in the way. This will be the ultimate test for the free enterprise system.
BTW...I do think there was running water there sometime in the past, but, if hydrogen can be detected...why not oxygen?
Not a stupid question at all!
(from the NASA web site:)
When exposed to cosmic rays (charged particles in space that come from the stars, including our sun), chemical elements in soils and rocks emit uniquely identifiable signatures of energy in the form of gamma rays. The gamma ray spectrometer (GRS) looks at these signatures, or energies, coming from the elements present in the Martian soil.
By measuring gamma rays coming from the Martian surface, it is possible to calculate how abundant various elements are and how they are distributed around the planet's surface. Gamma rays, emitted from the nuclei of atoms, show up as sharp emission lines on the instrument's spectrum. While the energy represented in these emissions determines which elements are present, the intensity of the spectrum reveals the elements concentrations.
How are gamma rays and neutrons produced by cosmic rays? Incoming cosmic rays--some of the highest-energy particles--collide with atoms in the soil. When atoms are hit with such energy, neutrons are released, which scatter and collide with other atoms. The atoms get " excited" in the process, and emit gamma rays to release the extra energy so they can return to their normal rest state. Some elements like potassium, uranium, and thorium are naturally radioactive and give off gamma rays as they decay, but all elements can be excited by collisions with cosmic rays to produce gamma rays. The HEND and Neutron Spectrometers on GRS directly detect scattered neutrons, and the Gamma Sensor detects the gamma rays.
How GRS Will Help Detect Water:
By measuring neutrons, it is possible to calculate the abundance of hydrogen on Mars, thus inferring the presence of water. The neutron detectors are sensitive to concentrations of hydrogen in the upper meter of the surface. Like a virtual shovel "digging into" the surface, the spectrometer will allow scientists to peer into this shallow subsurface of Mars and measure the amount of hydrogen that exists there. Since hydrogen is most likely present in the form of water ice, the spectrometer will be able to measure directly the amount of permanent ground ice and how it changes with the seasons.
Mere details, compared to the impediment of bureaucracy.
Excuse me, I may retire on Mars (or the Moon) someday. Don't ruin the neighborhood before I even get there!
I agree completely. Also I agree with this statement from Heinlein:
To what extent is civilization retarded by the laughing, jackassas, the empty-minded belittlers.
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